The Arecibo 327 MHz Drift-Scan Survey (ar327) published its results in papers published from 2013 to 2021 with a total of 45 new pulsars discovered. It detected a grand total of 4 pulsars. The fastest pulsar discovered was J2055+15 with a period of 2.16 milliseconds and the slowest pulsar was J1956+07 with a period of 5.01248 seconds.
The smallest pulsar dispersion measure was J2234+0611 with a DM of 10.7645 pc/cc and the largest pulsar dispersion measure was J1942+0147 with a DM of 133.3 pc/cc. There were a total of 2126 pulsars known before the first discovery was published. This survey increased the total amount of known pulsars by 2.0%.
There were 4 papers written about the discoveries of this survey: Goals, Strategies and First Discoveries of AO327, the Arecibo All-sky 327 MHz Drift Pulsar Survey, New Discoveries from the Arecibo 327 MHz Drift Pulsar Survey Radio Transient Search, Pulsar J1411+2551: A Low-mass Double Neutron Star System, The Discovery of Six Recycled Pulsars from the Arecibo 327 MHz Drift-Scan Pulsar Survey.
PSRs discovered by the Arecibo 327 MHz Drift-Scan Survey
| JNAME | SPIN PERIOD | DM | MAGNETIC FIELD STRENGTH |
|---|---|---|---|
| J0011+08 | 2.553 seconds | 24.9 pc/cc | * |
| J0050+03 | 1.367 seconds | 26.5 pc/cc | * |
| J0154+1833 | 2.365 milliseconds | 19.8 pc/cc | 8.41e+07 G |
| J0158+21 | 505.3 milliseconds | 20.0 pc/cc | * |
| J0229+20 | 806.9 milliseconds | 27.0 pc/cc | * |
| J0241+16 | 1.545 seconds | 16.0 pc/cc | * |
| J0244+14 | 2.128 seconds | 31.0 pc/cc | * |
| J0457+23 | 504.9 milliseconds | 59.0 pc/cc | * |
| J0550+09 | 1.745 seconds | 86.6 pc/cc | * |
| J0608+00 | 1.076 seconds | 48.5 pc/cc | * |
| J0611+04 | 1.674 seconds | 69.9 pc/cc | * |
| J0630+19 | 1.249 seconds | 48.1 pc/cc | * |
| J0806+08 | 2.063 seconds | 46.0 pc/cc | * |
| J0848+16 | 452.4 milliseconds | 38.0 pc/cc | * |
| J0928+06 | 2.06 seconds | 49.8 pc/cc | * |
| J1603+18 | 503.0 milliseconds | 29.7 pc/cc | * |
| J1656+00 | 1.498 seconds | 46.9 pc/cc | * |
| J1717+03 | 3.901 seconds | 25.6 pc/cc | * |
| J1720+00 | 3.357 seconds | 46.2 pc/cc | * |
| J1726-00 | 1.309 seconds | 57.0 pc/cc | * |
| J1738+04 | 1.392 seconds | 23.6 pc/cc | * |
| J1743+05 | 1.474 seconds | 56.1 pc/cc | * |
| J1749+16 | 2.312 seconds | 59.6 pc/cc | * |
| J1750+07 | 1.909 seconds | 55.4 pc/cc | * |
| J1802+03 | 664.3 milliseconds | 77.0 pc/cc | * |
| J1807+04 | 798.9 milliseconds | 53.0 pc/cc | * |
| J1854+36 | 1.3 seconds | 59.8 pc/cc | * |
| J1937-00 | 240.1 milliseconds | 68.6 pc/cc | * |
| J1938+14 | 2.903 seconds | 75.4 pc/cc | * |
| J1942+0147 | 1.405 seconds | 133.3 pc/cc | * |
| J1945+07 | 1.074 seconds | 62.0 pc/cc | * |
| J1946+14 | 2.282 seconds | 50.3 pc/cc | * |
| J1956+07 | 5.012 seconds | 61.3 pc/cc | * |
| J2055+15 | 2.16 milliseconds | 40.2 pc/cc | 2.11e+08 G |
| J2105+07 | 3.747 seconds | 52.6 pc/cc | * |
| J2329+16 | 632.1 milliseconds | 31.0 pc/cc | * |
| J2340+08 | 303.3 milliseconds | 24.0 pc/cc | * |
| JNAME | SPIN PERIOD | DM | MAGNETIC FIELD STRENGTH | ORBITAL PERIOD | ECCENTRICITY |
|---|---|---|---|---|---|
| J0453+1559 | 45.782 milliseconds | 30.31 pc/cc | 2.95e+09 G | 4.072 days | 0.113 |
| J0509+0856 | 4.056 milliseconds | 38.32 pc/cc | 1.35e+08 G | 4.908 days | 2.2e-05 |
| J0709+0458 | 34.429 milliseconds | 44.27 pc/cc | 3.66e+09 G | 4.367 days | 2.2e-04 |
| J0732+2314 | 4.09 milliseconds | 44.67 pc/cc | 1.59e+08 G | 30.23 days | 9.2e-06 |
| J0824+0028 | 9.861 milliseconds | 34.55 pc/cc | 1.22e+09 G | 23.207 days | 2.3e-04 |
| J1411+2551 | 62.453 milliseconds | 12.37 pc/cc | 2.47e+09 G | 2.616 days | 0.17 |
| J2204+2700 | 84.703 milliseconds | 35.07 pc/cc | 3.37e+09 G | 2.232 years | 1.5e-03 |
| J2234+0611 | 3.577 milliseconds | 10.76 pc/cc | 2.1e+08 G | 32.001 days | 0.129 |
PSRs detected by the Arecibo 327 MHz Drift-Scan Survey
| JNAME | SPIN PERIOD | DM | MAGNETIC FIELD STRENGTH |
|---|---|---|---|
| J0627+0649 | 346.523 milliseconds | 86.6 pc/cc | 7.76e+11 G |
| J1821+0155 | 33.781 milliseconds | 51.75 pc/cc | 1e+09 G |
| J2251+24 | 1.798 seconds | 34.6 pc/cc | * |
| J2347+02 | 1.383 seconds | 15.0 pc/cc | * |